Fig. 4

Reconstructed images from the MUSE data cube. Each panel shows the host of GRB 980425 in a different nebular line. Top left: Hα. Top right: [O iii](λ5007). Bottom left: [S ii](λ6731). Bottom right: [S iii](λ9070). All panels are approximately 55′′ by 55′′, or 10 kpc by 10 kpc at the GRB redshift. The effective spatial resolution is given by the point spread function (PSF) indicated in the lower left corner of each image with a full width half maximum (FWHM) of approximately 0.′′9 or 160 pc.
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